activity
20062026
most citedSPCANet: Stellar Parameters and Chemical Abundances Network for LAMOST-II Medium Resolution Survey

67 citations · 273 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.SR2026

Weighing Hidden Companions of Compact Object Candidates via Rotational Broadening

Rui Wang, Zhi-Xiang Zhang, Wei-Min Gu +3

The determination of unseen companion masses () is essential for identifying compact objects in binary systems, yet obtaining reliable orbital inclinations remains one of the…

astro-ph.IM2025

Mock Observations for the CSST Mission: Main Surveys-the Slitless Spectroscopy Simulation

Xin Zhang, Yue-dong Fang, Cheng-liang Wei +14

The China Space Station Telescope (CSST), slated to become China's largest space-based optical telescope in the coming decade, is designed to conduct wide-field sky surveys with hi…

astro-ph.SR2023

Stellar Atmospheric Parameters for Cool Dwarfs in Gaia DR3

Cai-Xia Qu, A-Li Luo, Rui Wang +4

We provide a catalogue of atmospheric parameters for 1,806,921 cool dwarfs from Gaia DR3 which lie within the range covered by LAMOST cool dwarf spectroscopic parameters: 3200 K <…

astro-ph.SR2023★ 21 cited

Stellar Parameters and Chemical Abundances Estimated from LAMOST-II DR8 MRS based on Cycle-StarNet

Rui Wang, A-Li Luo, Shuo Zhang +3

Deriving stellar atmospheric parameters and chemical abundances from stellar spectra is crucial for understanding the evolution of the Milky Way. By performing a fitting with MARCS…

astro-ph.SR2022★ 3 cited

M Subdwarf Research III. Spectroscopic Diagnostics for Breaking Parameter Degeneracy

Shuo Zhang, Hua-Wei Zhang, Georges Comte +5

To understand the parameter degeneracy of M subdwarf spectra at low resolution, we assemble a large number of spectral features in the wavelength range of 0.6-2.5 μm with band stre…

astro-ph.SR2022★ 1 cited

A Spectroscopic Modelling Method for the Detached Eclipsing Binaries to Derive Atmospheric Parameters

Xiang-Lei Chen, A-Li Luo, Jian-Jun Chen +5

Based on luminosity contributions, we develop a spectroscopic modelling method to derive atmospheric parameters of component stars in binary systems. The method is designed for tho…